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Title: NEAR-INFRARED SPECTROSCOPY OF THE BLUE COMPACT DWARF GALAXY MARKARIAN 59

Journal Article · · Astrophysical Journal
 [1];
  1. Main Astronomical Observatory, Ukrainian National Academy of Sciences, 27 Zabolotnoho Str., Kyiv 03680 (Ukraine)

We present near-infrared (NIR) spectroscopic observations of the blue compact dwarf (BCD) galaxy Markarian 59 (Mrk 59), obtained with the TripleSpec spectrograph mounted on the 3.5 m Apache Point Observatory telescope. The NIR spectrum of Mrk 59, which covers the 0.90 {mu}m-2.40 {mu}m wavelength range, shows atomic hydrogen, molecular hydrogen, helium, sulfur, and iron emission lines. The NIR data have been supplemented by a Sloan Digital Sky Survey optical spectrum. We found extinction in the BCD to be low (A(V) = 0.24 mag) and to be the same in both the optical and NIR ranges. The NIR light does not reveal hidden star formation. The H{sub 2} emission comes from dense clumps and the H{sub 2} vibrational emission-line intensities can be accounted for by photon excitation. No shock excitation is needed. A CLOUDY photoionization model of Mrk 59 reproduces well the observed optical and NIR emission-line fluxes. There is no need to invoke sources of ionization other than stellar radiation. The [Fe II] 1.257 and 1.643 {mu}m emission lines, often used as supernova shock indicators in low-excitation high-metallicity starburst galaxies, cannot play such a role in high-excitation low-metallicity H II regions such as Mrk 59.

OSTI ID:
21371835
Journal Information:
Astrophysical Journal, Vol. 703, Issue 2; Other Information: DOI: 10.1088/0004-637X/703/2/1984; ISSN 0004-637X
Country of Publication:
United States
Language:
English